Spectroscopy and Spectral Analysis, Volume. 43, Issue 6, 1875(2023)
Automatic Classification Method of Star Spectra Based on Semi-Supervised Mode
[1] [1] Li Xiangru, Pan Ruyang, Duan Fuqing. Research in Astronomy and Astrophysics, 2017, 17(4): 36.
[2] [2] Morgan W, Keenan P. Annual Review of Astronomy and Astrophysics, 1973, 11: 29.
[3] [3] Du Bing, Luo A-li, Zhang Shuo, et al. Research in Astronomy and Astrophysics, 2021, 21(8): 202.
[4] [4] Fan J, Han F, Liu H. Nationanl Science Review, 2014, 1(2): 293.
[5] [5] Schierscher F, Paunzen E. Astronomische Nachrichten, 2011, 332(6): 597.
[6] [6] Liu C, Cui W Y, Zhang B, et al. Research in Astronomy and Astrophysics, 2015, 15(8): 1137.
[7] [7] Kheirdastan S, Bazarghan M. Astrophysics and Space Science, 2016, 361(9): 304.
[11] [11] Du Changde, Luo Ali, Yang Haifeng. New Astronomy, 2017, 51: 51.
[12] [12] Zheng Zipeng, Qiu Bo, Luo A-li, et al. Publications of the Astronomical Society of the Pacific, 2020, 132: 024504.
[13] [13] Si Jianmin, Li Yinbi, Luo A-li, et al. Research in Astronomy and Astrophysics, 2015, 15(10): 1671.
Get Citation
Copy Citation Text
JIANG Xia, QIU Bo, WANG Lin-qian, GUO Xiao-yu. Automatic Classification Method of Star Spectra Based on Semi-Supervised Mode[J]. Spectroscopy and Spectral Analysis, 2023, 43(6): 1875
Received: Mar. 18, 2022
Accepted: --
Published Online: Jan. 8, 2024
The Author Email: